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Numerical Simulation of the Dynamics of Turbulent Swirling Flames

Numerical Simulation of the Dynamics of Turbulent Swirling Flames

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2.2 The Energy Spectrum and <strong>Turbulent</strong> Length Scales<br />

The kinetic energy (per unit mass) produced by <strong>the</strong> instantaneous velocity turbulent<br />

fluctuations is defined by:<br />

k ≡ 1 2 u′ i u′ i = 1 2<br />

(<br />

u ′ x 2 + u ′ y 2 + u ′ z<br />

2 ) . (2.5)<br />

The mean value <strong>of</strong> <strong>the</strong> instantaneous kinetic energy <strong>of</strong> <strong>the</strong> turbulent fluctuations<br />

is called <strong>the</strong> turbulent kinetic energy [164] and defined by:<br />

〈k〉 ≡ 1 2<br />

〈 〉<br />

u<br />

′<br />

1<br />

(〈 〉 〈 〉 〈 〉)<br />

i u′ i = u ′ 2<br />

x + u ′ 2<br />

y + u ′ 2<br />

z . (2.6)<br />

2<br />

2.2 The Energy Spectrum and <strong>Turbulent</strong> Length Scales<br />

Eddies with various length scales are present in turbulent flows producing<br />

different amounts <strong>of</strong> kinetic energy. An example to illustrate <strong>the</strong> variation <strong>of</strong><br />

scales in a turbulent flow is shown in Figs. 2.2 and 2.3. Inside <strong>the</strong> flow, <strong>the</strong><br />

eddies are mixed and continually forming and breaking down. In this process,<br />

<strong>the</strong> largest scale eddies interact with and extract energy from <strong>the</strong> mean flow<br />

mainly by vortex stretching (due to mean velocity gradients) [201, 208] and<br />

transfer it to <strong>the</strong> smaller scales. The large eddies break down into smaller ones,<br />

which break down into yet smaller eddies, until <strong>the</strong>y become small enough<br />

that viscous dissipation effects dominate and simply dissipate into internal<br />

energy [130]. This concept, known also as <strong>the</strong> energy cascade, was introduced<br />

by Richardson in 1922 [170]. He summarized this process with <strong>the</strong> following<br />

verse:<br />

Big whorls have little whorls,<br />

Which feed on <strong>the</strong>ir velocity,<br />

And little whorls have lesser whorls,<br />

And so on to viscosity.<br />

From <strong>the</strong> concept <strong>of</strong> energy cascade, <strong>the</strong> turbulent kinetic energy (Eq. (2.6))<br />

depends on <strong>the</strong> energy produced by <strong>the</strong> different eddies. The contribution<br />

<strong>of</strong> <strong>the</strong> different scales on <strong>the</strong> turbulent kinetic energy can be defined by its<br />

spectrum in wave number space E(κ). Then <strong>the</strong> turbulent kinetic energy is<br />

11

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